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20012009
most citedCalFUSE v3: A Data-Reduction Pipeline for the Far Ultraviolet Spectroscopic Explorer

112 citations · 375 across the 7 of their papers we have counts for

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astro-ph200821 cited

The radius and other fundamental parameters of the F9 V star beta Virginis

J. R. North, J. Davis, J. G. Robertson +10

We have used the Sydney University Stellar Interferometer (SUSI) to measure the angular diameter of the F9 V star beta Virginis. After correcting for limb darkening and combining w…

astro-ph200827 cited

Characterization of integrated optics components for the second generation of VLTI instruments

S. Lacour, L. Jocou, T. Moulin +10

Two of the three instruments proposed to ESO for the second generation instrumentation of the VLTI would use integrated optics for beam combination. Several design are studied, inc…

astro-ph200872 cited

GRAVITY: getting to the event horizon of Sgr A*

F. Eisenhauer, G. Perrin, W. Brandner +45

We present the second-generation VLTI instrument GRAVITY, which currently is in the preliminary design phase. GRAVITY is specifically designed to observe highly relativistic motion…

astro-ph200750 cited

The Keck Aperture Masking Experiment: Multi-Wavelength Observations of 6 Mira Variables

H. C. Woodruff, P. G. Tuthill, J. D. Monnier +5

The angular diameters of six oxygen rich Mira-type long-period variables have been measured at various near-infrared (NIR) wavelengths using the aperture masking technique in an ex…

astro-ph2007112 cited

CalFUSE v3: A Data-Reduction Pipeline for the Far Ultraviolet Spectroscopic Explorer

W. V. Dixon, D. J. Sahnow, P. E. Barrett +13

Since its launch in 1999, the Far Ultraviolet Spectroscopic Explorer (FUSE) has made over 4600 observations of some 2500 individual targets. The data are reduced by the Principal I…

astro-ph200642 cited

High dynamic range imaging by pupil single-mode filtering and remapping

G. Perrin, S. Lacour, J. Woillez +1

Because of atmospheric turbulence, obtaining high angular resolution images with a high dynamic range is difficult even in the near infrared domain of wavelengths. We propose a nov…